PDS_VERSION_ID                    = PDS3
LABEL_REVISION_NOTE               = "2017-04-27 Initial"
RECORD_TYPE                       = STREAM
SPACECRAFT_NAME                   = "JUNO"
TARGET_NAME                       = "JUPITER"

OBJECT                            = DATA_SET_MAP_PROJECTION
 DATA_SET_ID                      = "JUNO-J-JUNOCAM-4-RDR-L1B-V1.0"
 OBJECT                           = DATA_SET_MAP_PROJECTION_INFO
  MAP_PROJECTION_TYPE             = "SIMPLE CYLINDRICAL"
  MAP_PROJECTION_DESC             = "

    In the simple cylindrical projection [SNYDER1987], parallels
    of latitude and meridians of longitude are straight lines that
    intersect one another at right angles.

    Images in this projection are centered on the equator. Map
    resolution is constant throughout the image, thus increasing
    distortion away from the poles.

    The transformation from latitude and longitude (LAT, LON) in
    degrees to LINE and SAMPLE is given by the following equations.

    SCALE = MAP_RESOLUTION

    SAMPLE = SAMPLE_PROJECTION_OFFSET+SCALE*(LON-CENTER_LONGITUDE)+1

    LINE = LINE_PROJECTION_OFFSET-SCALE*(LAT-CENTER_LATITUDE)+1

    In the above definitions, integral values of LINE and SAMPLE
    correspond to the center of a pixel, and the top left image
    pixel has LINE=1 and SAMPLE=1. LAT and LON are the latitude and
    longitude of a given spot on the surface in degrees.

    LINE_PROJECTION_OFFSET
      is the image line number minus one on which the map projection
      origin occurs.  The map projection origin is the intersection
      of the equator and the projection longitude CENTER_LONGITUDE.

    SAMPLE_PROJECTION_OFFSET
      is the sample number minus one on which the map projection
      origin occurs.

    CENTER_LATITUDE
      is the value of the projection latitude in degrees, which is
      typically the latitude that passes through the center of the
      projection.

    CENTER_LONGITUDE
      is the value of the projection longitude in degrees, which is
      typically the longitude that passes through the center of the
      projection.

    MAP_RESOLUTION
      is the number of pixels per degree at the projection origin.

    For these products, Jupiter System 3 longitude and planetographic
    latitude are used.  The prime meridian is defined per Archinal et al,
    'Report of the IAU Working Group on Cartographic Coordinates
    and Rotational Elements: 2009 [ARCHINAL2010].'
  "

  ROTATIONAL_ELEMENT_DESC         = "IAU2009"

  OBJECT                          = DS_MAP_PROJECTION_REF_INFO
   REFERENCE_KEY_ID               = "SNYDER1987"
  END_OBJECT                      = DS_MAP_PROJECTION_REF_INFO

  OBJECT                          = DS_MAP_PROJECTION_REF_INFO
   REFERENCE_KEY_ID               = "ARCHINAL2010"
  END_OBJECT                      = DS_MAP_PROJECTION_REF_INFO

 END_OBJECT                       = DATA_SET_MAP_PROJECTION_INFO

END_OBJECT                        = DATA_SET_MAP_PROJECTION

END